collaborators

5 papers

astro-ph.HE2025

The very high X-ray polarisation of accreting black hole IGRJ17091-3624 in the hard state

Melissa Ewing, Maxime Parra, Guglielmo Mastroserio +26

We report the first detection of the X-ray polarisation of the transient black hole X-ray binary IGRJ17091-3624 taken with the Imaging X-ray polarimetry Explorer (IXPE) in March 20…

astro-ph.CO2025

Constraining gas motion and non-thermal pressure beyond the core of the Abell 2029 galaxy cluster with XRISM

XRISM Collaboration, Marc Audard, Hisamitsu Awaki +137

We report a detailed spectroscopic study of the gas dynamics and hydrostatic mass bias of the galaxy cluster Abell 2029, utilizing high-resolution observations from XRISM Resolve.…

astro-ph.HE2025

Supermassive Black Holes in X-rays: From Standard Accretion to Extreme Transients

Erin Kara, Javier García

X-rays are a critical wavelength for understanding supermassive black holes (SMBHs). X-rays probe the inner accretion flow, closest to the event horizon, where gas inspirals, relea…

astro-ph.GA2025

Frequency-resolved time lags due to X-ray disk reprocessing in AGN

Christos Panagiotou, Iossif Papadakis, Erin Kara +6

Over the last years, a number of broadband reverberation mapping campaigns have been conducted to explore the short-term UV and optical variability of nearby AGN. Despite the exten…

physics.flu-dyn2024

A second-generation URANS model (STRUCT) applied to a Generic Side Mirror and its Impact on Sound Generation

Jorge Munoz-Paniagua, Javier García, Eduardo Latorre-Iglesias

A generic side mirror can be approximated to the combination of a half cylinder topped with a quarter of sphere. The flow structure in the wake of the side mirror is highly transie…